Solar gravity modes from ACRIM/SMM irradiance data

Details Solar gravity modes from ACRIM/SMM irradiance data Solar gravity modes from ACRIM/SMM irradiance data

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mmsai..55...99f&link_type=abstract

(European Physical Society, Ministero della Pubblica Istruzione, and Universita di Catania, EPS Study Conference on Oscillations

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16

Irradiance, Solar Gravitation, Solar Maximum Mission, Solar Oscillations, Vibration Mode, Power Spectra, Radiometers

Scientific paper

The record of 280 days of continuous data of the ACRIM radiometer on board the Solar Maximum Mission satellite is analyzed in the frequency range 2-80 microhertz. Gravity modes of degree one and two with orders from about 10 to several hundred can be localized. Due to the complexity of the spectrum of the enormous number of lines in a given frequency interval, the individual identification is very difficult. A statistical method to determine the fundamental period and the rate of rotation as seen by rotational splitting is described, and the results compared with other determinations.

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